48 |
|
.TP |
49 |
|
.BR \-o |
50 |
|
Print original values, before exposure compensation. |
51 |
+ |
If the input file is in XYZE format, the Y (green) channel |
52 |
+ |
will correspond to units of candelas/meter^2. |
53 |
+ |
Otherwise, the RGB values should be in spectral watts/steradian/meter^2. |
54 |
|
Specifying |
55 |
|
.I \+o |
56 |
< |
uses final values, which is the default. |
56 |
> |
uses final exposed values, which is the default. |
57 |
|
.TP |
58 |
|
.BR \-h |
59 |
|
Do not print header. |
210 |
|
x or along y. |
211 |
|
Most Radiance pictures are sorted top to bottom, then left |
212 |
|
to right. |
213 |
< |
This corresponds to a specification of the form "-y yres +x xres". |
213 |
> |
This corresponds to a specification of the form "\-y yres +x xres". |
214 |
|
Either an upper or lower case 'X' may be used for this option. |
215 |
|
Like the |
216 |
|
.I \-y |
220 |
|
.SH EXAMPLE |
221 |
|
To look at the original, unique pixels in picture: |
222 |
|
.IP "" .2i |
223 |
< |
pvalue -o -u picture | more |
223 |
> |
pvalue \-o \-u picture | more |
224 |
|
.PP |
225 |
|
To convert from a 512x400 8-bit greyscale image in bottom to top, |
226 |
|
left to right scanline ordering: |
227 |
|
.IP "" .2i |
228 |
< |
pvalue -r -db -b -h +y 400 +x 512 input.im > flipped.pic |
228 |
> |
pvalue \-r \-db \-b \-h +y 400 +x 512 input.im > flipped.pic |
229 |
|
.br |
230 |
< |
pflip -v flipped.pic > final.pic |
230 |
> |
pflip \-v flipped.pic > final.pic |
231 |
|
.SH AUTHOR |
232 |
|
Greg Ward |
233 |
|
.SH BUGS |